Radial Velocity and Light Curves Analysis of the Contact Binary V1073 Cygni

Details Radial Velocity and Light Curves Analysis of the Contact Binary V1073 Cygni Radial Velocity and Light Curves Analysis of the Contact Binary V1073 Cygni

Dec 2006

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2006ap%26ss.306...29j&link_type=abstract

Astrophysics and Space Science, Volume 306, Issue 1-2, pp. 29-32

Astronomy and Astrophysics

Astrophysics

1

Stars, Variable, Binaries, Eclipsing Binary, Individual, V1073 Cygni

Scientific paper

In this study complete BV light curves of the W Ursae Majoris binary V1073 Cygni obtained in 2005 are presented. We have used the spectroscopic data of V1073 Cyg obtained by Ahn et al. (1992) for analysis. The analysis of radial velocity and light curves was made with Wilson} program (1998) and the geometric and physical elements} of the system were derived. By searching the simultaneous} solutions of the system, we have determined the masses and radii of the components: 1.64M&sun;, 2.275R&sun; for the primary component and 0.55M&sun;, 1.397R&sun; for the secondary component respectively. The effective temperature of 6494 ± 53 K for the secondary component was also estimated.

Affiliated with

Also associated with

No associations

Rating

Radial Velocity and Light Curves Analysis of the Contact Binary V1073 Cygni does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.

If you have personal experience with Radial Velocity and Light Curves Analysis of the Contact Binary V1073 Cygni, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Radial Velocity and Light Curves Analysis of the Contact Binary V1073 Cygni will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1239077